991 resultados para upwind compact difference scheme


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A new finite-difference scheme is presented for the second derivative of a semivectorial field in a step-index optical waveguide with tilt interfaces. The present scheme provides an accurate description of the tilt interface of the nonrectangular structure. Comparison with previously presented formulas shows the effectiveness of the present scheme.

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Starting from nonhydrostatic Boussinesq approximation equations, a general method is introduced to deduce the dispersion relationships. A comparative investigation is performed on inertia-gravity wave with horizontal lengths of 100, 10 and 1 km. These are examined using the second-order central difference scheme and the fourth-order compact difference scheme on vertical grids that are currently available from the perspectives of frequency, horizontal and vertical component of group velocity. These findings are compared to analytical solutions. The obtained results suggest that whether for the second-order central difference scheme or for the fourth-order compact difference scheme, Charny-Phillips and Lorenz ( L) grids are suitable for studying waves at the above-mentioned horizontal scales; the Lorenz time-staggered and Charny-Phillips time staggered (CPTS) grids are applicable only to the horizontal scales of less than 10 km, and N grid ( unstaggered grid) is unsuitable for simulating waves at any horizontal scale. Furthermore, by using fourth-order compact difference scheme with higher difference precision, the errors of frequency and group velocity in horizontal and vertical directions produced on all vertical grids in describing the waves with horizontal lengths of 1, 10 and 100 km cannot inevitably be decreased. So in developing a numerical model, the higher-order finite difference scheme, like fourth-order compact difference scheme, should be avoided as much as possible, typically on L and CPTS grids, since it will not only take many efforts to design program but also make the calculated group velocity in horizontal and vertical directions even worse in accuracy.

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Nonlinear phenomena play an essential role in the sound production process of many musical instruments. A common source of these effects is object collision, the numerical simulation of which is known to give rise to stability
issues. This paper presents a method to construct numerical schemes that conserve the total energy in simulations of one-mass systems involving collisions, with no conditions imposed on any of the physical or numerical parameters.
This facilitates the adaptation of numerical models to experimental data, and allows a more free parameter adjustment in sound synthesis explorations. The energy preservedness of the proposed method is tested and demonstrated though several examples, including a bouncing ball and a non-linear oscillator, and implications regarding the wider applicability are discussed.

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An efficient finite difference scheme is presented for the inviscid terms of the three-dimensional, compressible flow equations for chemical non-equilibrium gases. This scheme represents an extension and an improvement of one proposed by the author, and includes operator splitting.

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We present a finite difference scheme, with the TVD (total variation diminishing) property, for scalar conservation laws. The scheme applies to non-uniform meshes, allowing for variable mesh spacing, and is without upstream weighting. When applied to systems of conservation laws, no scalar decomposition is required, nor are any artificial tuning parameters, and this leads to an efficient, robust algorithm.

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A finite difference scheme is presented for the inviscid terms of the equations of compressible fluid dynamics with general non-equilibrium chemistry and internal energy.

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A finite difference scheme is presented for the solution of the two-dimensional equations of steady, supersonic, compressible flow of real gases. The scheme incorparates numerical characteristic decomposition, is shock-capturing by design and incorporates space-marching as a result of the assumption that the flow is wholly supersonic in at least one space dimension. Results are shown for problems involving oblique hydraulic jumps and reflection from a wall.

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En el presente artículo se muestran las ventajas de la programación en paralelo resolviendo numéricamente la ecuación del calor en dos dimensiones a través del método de diferencias finitas explícito centrado en el espacio FTCS. De las conclusiones de este trabajo se pone de manifiesto la importancia de la programación en paralelo para tratar problemas grandes, en los que se requiere un elevado número de cálculos, para los cuales la programación secuencial resulta impracticable por el elevado tiempo de ejecución. En la primera sección se describe brevemente los conceptos básicos de programación en paralelo. Seguidamente se resume el método de diferencias finitas explícito centrado en el espacio FTCS aplicado a la ecuación parabólica del calor. Seguidamente se describe el problema de condiciones de contorno y valores iniciales específico al que se va a aplicar el método de diferencias finitas FTCS, proporcionando pseudocódigos de una implementación secuencial y dos implementaciones en paralelo. Finalmente tras la discusión de los resultados se presentan algunas conclusiones. In this paper the advantages of parallel computing are shown by solving the heat conduction equation in two dimensions with the forward in time central in space (FTCS) finite difference method. Two different levels of parallelization are consider and compared with traditional serial procedures. We show in this work the importance of parallel computing when dealing with large problems that are impractical or impossible to solve them with a serial computing procedure. In the first section a summary of parallel computing approach is presented. Subsequently, the forward in time central in space (FTCS) finite difference method for the heat conduction equation is outline, describing how the heat flow equation is derived in two dimensions and the particularities of the finite difference numerical technique considered. Then, a specific initial boundary value problem is solved by the FTCS finite difference method and serial and parallel pseudo codes are provided. Finally after results are discussed some conclusions are presented.

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Direct numerical simulation (DNS) is used to study flow characteristics after interaction of a planar shock with a spherical media interface in each side of which the density is different. This interfacial instability is known as the Richtmyer-Meshkov (R-M) instability. The compressible Navier-Stoke equations are discretized with group velocity control (GVC) modified fourth order accurate compact difference scheme. Three-dimensional numerical simulations are performed for R-M instability installed passing a shock through a spherical interface. Based on numerical results the characteristics of 3D R-M instability are analysed. The evaluation for distortion of the interface, the deformation of the incident shock wave and effects of refraction, reflection and diffraction are presented. The effects of the interfacial instability on produced vorticity and mixing is discussed.

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对运用迎风紧致格式求解非线性方程时混淆误差产生的机理进行了研究,通过算例对五阶迎风紧致格式与谱方法进行了比较,发现在混淆误差的处理上迎风紧致格式优于谱方法。

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通过直接数值模拟(DNS)研究槽道湍流的性质和机理。包含五个部分:1)湍流直接数值模拟的差分方法研究。2)求解不可压N-S方程的高效算法和不可压槽道湍流的直接数值模拟。3)可压缩槽道湍流的直接数值模拟和压缩性机理分析。4)“二维湍流”的机理分析。5)槽道湍流的标度律分析。1.针对壁湍流计算网格变化剧烈的特点,构造了基于非等距网格的的迎风紧致格式。该方法直接针对计算网格构造格式中的系数,克服了传统方法采用 Jacobian 变换因网格变化剧烈而带来的误差。针对湍流场的多尺度特性分析了差分格式的精度、网格尺度与数值模拟能分辨的最小尺度的关系,给出不同差分格式对计算网格步长的限制。同时分析了计算中混淆误差的来源和控制方法,指出了迎风型紧致格式能很好地控制混淆误差。2.将上述格式与三阶精度的Adams半隐格式相结合,构造了不可压槽道湍流直接数值模拟的高效算法。该算法利用基于交错网格的离散形式的压力Poisson方程求解压力项,避免了压力边界条件处理的困难。利用FFT对方程中的隐式部分进行解耦,解耦后的方程采用追赶法(LU分解法)求解,大大减少了计算量。为了检验该方法,进行了三维不可压槽道湍流的直接数值模拟,得到了Re=2800的充分发展不可压槽道湍流,并对该湍流场进行了统计分析。包括脉动速度偏斜因子在内的各阶统计量与实验结果及Kim等人的计算结果吻合十分理想,说明本方法是行之有效的。3.进行了三维充分发展的可压缩槽道湍流的直接数值模拟。得到了 Re=3300,Ma=0.8的充分发展可压槽道湍流的数据库。流场的统计特征(如等效平均速度分布,“半局部”尺度无量纲化的脉动速度均方根)和他人的数值计算结果吻合。得到了可压槽道湍流的各阶统计量,其中脉动速度的偏斜因子和平坦因子等高阶统计量尚未见其他文献报道。同时还分析了压缩性效应对壁湍流影响的机理,指出近壁处的压力-膨胀项将部分湍流脉动的动能转换成内能,使得可压湍流近壁速度条带结构更加平整。4.模拟了二维不可压槽道流动的饱和态(所谓“二维湍流”),分析了“二维槽道湍流”的非线性行为特征。分析了流场中的上抛-下扫和间歇现象,研究了“二维湍流”与三维湍流的区别。指出“二维湍流”反映了三维湍流的部分特征,同时指出了展向扰动对于湍流核心区发展的重要性。5.首次对可压缩槽道湍流及“二维槽道湍流”标度律进行了分析,得出了以下结论:a)槽道湍流中,在槽道中心线附近较宽的区域,存在标度律。b)该区域流场存在扩展自相似性(ESS)。c)在Mach数不是很高时,压缩性对标度指数影响不大。本文结果同SL标度律的理论值吻合较好,有效支持了该理论。对“二维槽道湍流”也有相似的结论,但与三维湍流不同的是,“二维槽道湍流”存在标度律的区域更宽,近壁处的标度指数比中心处有所升高。

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可压平面混合层是包含复杂多时空尺度运动的非定常流体力学部问题,具有深刻的理论意义和广泛的应用背景。针对该问题所涉及内容的多面性,本文的目的是,基于高精度、高分辨率数值算法的构造、发展和数值行为分析,采用线性稳定性分析和直接数值模拟方法。从理论和计算两方面集中研究压缩性效应、粘性效应、初值效应以及燃烧反应放热效应等对可压平面混合层早期稳定性行为和大尺度拟序涡结构非线性演化的影响。以混合层已有研究成果的分析和综述为开端,论文主体共包括四部分:第一部分是可压平面混合层时间/空间模式数值线性稳定性分析。实现了高精度对称紧致差分格式(SCD)对可压粘性扰动线性稳定性边值问题的求解,对导出的线性和非线性离散特征值问题,提出了两个高效局部解法。研究涉及二维/三维扰动波、无粘/粘性扰动波、特征函数和特征值谱、第一/第二模态、超声速快/慢模态、速度比和密度比等。验证了对流Mach数Mc为一个合理的压缩性参数。指出压缩性效应和粘性效应对最不稳定扰动波的波数(频率)和增长率呈相拟的抑制作用,且时间模式稳定性分析结果在许多方面是可信的。从随机和线性扰动场出发,采用高精度五阶迎风紧致和六阶对称紧致混合差分算法(UCD5/SCD6)对可压平面混合层的稳定性特征进行了直接数值模拟,揭示了初始主导线性扰动与一些实际涡结构非线性作用形态间的内在关联,印证了线性稳定性分析方法的合理性和有效性。第二部分是高精度迎风紧致差分格式(UCD)时空全离散数值行为分析。导出了其一维/二维一般色散表达式。研究表明,UCD格式在高波数区具有内在的全离散耗散和色散特性;其数值群速度的快/慢特征可因CFL数不同而改变;在稳定CFL数下简单附加人工粘性可强化UCD格式在高波数区的耗散量;提高时间精度可放宽稳定CFL数限制;UCD格式的二维全离散色散介质中存在三个不同性质的数值波,其全离散稳定性由数值声波主控。第三部分实现了高精度UCD5/SCD6差分算法对空间发展可压平面混合层的直接数值模拟。通过亚谐扰动波的个数和扰动频率的控制,捕捉到了基频涡的饱和、一次和二次对并等现象,显示了大尺度涡结构与入中初始扰动方式之间的内在联系。利用参数Mc观察了压缩性效应对大尺度涡空间演化及其相互作用的影响。第四部分实现了高精度UCD5/SCD6差分算法对非预混扩散火焰化学反应平面混合层的直接数值模拟。研究指出,放热效应可抑制和延迟涡的形成,使基频涡卷拉伸甚至丧失,混合层Reynolds 应力ρu'v'和流向速度波动关联项u'v'下降,以致涡结构与外流动量交换和标量输运减少,脉动输运能力被削弱,从而混合效率、产物生成率和混合层增长率下降,放热主要通过膨胀效应和斜压效应来抑制大尺度涡的演化。

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Non-standard finite difference methods (NSFDM) introduced by Mickens [Non-standard Finite Difference Models of Differential Equations, World Scientific, Singapore, 1994] are interesting alternatives to the traditional finite difference and finite volume methods. When applied to linear hyperbolic conservation laws, these methods reproduce exact solutions. In this paper, the NSFDM is first extended to hyperbolic systems of conservation laws, by a novel utilization of the decoupled equations using characteristic variables. In the second part of this paper, the NSFDM is studied for its efficacy in application to nonlinear scalar hyperbolic conservation laws. The original NSFDMs introduced by Mickens (1994) were not in conservation form, which is an important feature in capturing discontinuities at the right locations. Mickens [Construction and analysis of a non-standard finite difference scheme for the Burgers–Fisher equations, Journal of Sound and Vibration 257 (4) (2002) 791–797] recently introduced a NSFDM in conservative form. This method captures the shock waves exactly, without any numerical dissipation. In this paper, this algorithm is tested for the case of expansion waves with sonic points and is found to generate unphysical expansion shocks. As a remedy to this defect, we use the strategy of composite schemes [R. Liska, B. Wendroff, Composite schemes for conservation laws, SIAM Journal of Numerical Analysis 35 (6) (1998) 2250–2271] in which the accurate NSFDM is used as the basic scheme and localized relaxation NSFDM is used as the supporting scheme which acts like a filter. Relaxation schemes introduced by Jin and Xin [The relaxation schemes for systems of conservation laws in arbitrary space dimensions, Communications in Pure and Applied Mathematics 48 (1995) 235–276] are based on relaxation systems which replace the nonlinear hyperbolic conservation laws by a semi-linear system with a stiff relaxation term. The relaxation parameter (λ) is chosen locally on the three point stencil of grid which makes the proposed method more efficient. This composite scheme overcomes the problem of unphysical expansion shocks and captures the shock waves with an accuracy better than the upwind relaxation scheme, as demonstrated by the test cases, together with comparisons with popular numerical methods like Roe scheme and ENO schemes.

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For solving complex flow field with multi-scale structure higher order accurate schemes are preferred. Among high order schemes the compact schemes have higher resolving efficiency. When the compact and upwind compact schemes are used to solve aerodynamic problems there are numerical oscillations near the shocks. The reason of oscillation production is because of non-uniform group velocity of wave packets in numerical solutions. For improvement of resolution of the shock a parameter function is introduced in compact scheme to control the group velocity. The newly developed method is simple. It has higher accuracy and less stencil of grid points.